Effect of initial energy of hydrogen atoms on trapping and reaction in solid methane at 4 K

1982 ◽  
Vol 86 (10) ◽  
pp. 1781-1784 ◽  
Author(s):  
Akihiro Wakahara ◽  
Tetsuo Miyazaki ◽  
Kenji Fueki
1983 ◽  
Vol 87 (9) ◽  
pp. 1611-1613 ◽  
Author(s):  
Tetsuo Miyazaki ◽  
Haruyuki Tsuruta ◽  
Kenji Fueki

1982 ◽  
Vol 86 (19) ◽  
pp. 3881-3883 ◽  
Author(s):  
Tetsuo Miyazaki ◽  
Akihiro Wakahara ◽  
Takahiro Usui ◽  
Kenji Fueki

1960 ◽  
Vol 38 (10) ◽  
pp. 1722-1733 ◽  
Author(s):  
Michael Henchman ◽  
David Urch ◽  
Richard Wolfgang

The chemistry of hot hydrogen atoms has been studied using tritium of high kinetic energy as produced by nuclear recoil. The possibilities and limitations of this technique are discussed using a collision theory for reactions of atoms having a very high initial energy. Using this theory and certain experimental data, it is concluded that hot hydrogen atoms react to combine with organic molecules at very high collision efficiency (of the order of approximately 0.2 to 0.4) in the energy range 3–10 ev. There is no indication that collisions at much higher energies lead to combination. With most systems, e.g. alkanes, a wide variety of reactions is observed. The systematics of these hot reactions is discussed and evidence on their detailed mechanism is presented. It appears that most products are formed by a fast displacement of an atom or group by the hot hydrogen. There is no evidence for the formation of a common, internally equilibrated, collision complex which decays on a statistically determined basis to the various products. Instead, the course of the reactions seems largely governed by the direction and point of impact of the hot atom. Thus, stereochemical evidence indicates that axial approach of the hot hydrogen atom along the C—H bond axis leads to abstraction while approach at large angles to this axis results in displacement without Walden inversion. In some cases sufficient excitation energy is introduced in the hot displacement process to cause further decomposition of the primary product. This model of high-energy reactions is compared with that of thermal reactions and its general implications are briefly discussed.


1967 ◽  
Vol 31 ◽  
pp. 91-93 ◽  
Author(s):  
G. Herzberg

It is suggested that the diffuse interstellar lines are produced in the interstellar gas by molecules consisting of a few hydrogen atoms and one other atom, such as CH4+ or NH4. Diffuseness of the lines is assumed to result from predissociation of these molecules.


1979 ◽  
Vol 40 (C7) ◽  
pp. C7-479-C7-480 ◽  
Author(s):  
V. G. Dudnikov ◽  
G. I. Fiksel'

2002 ◽  
Vol 715 ◽  
Author(s):  
T. Su ◽  
Robin Plachy ◽  
P. C. Taylor ◽  
S. Stone ◽  
G. Ganguly ◽  
...  

AbstractWe study the H NMR line shapes of a sample of a-Si:H under several conditions: 1) as grown, 2) light-soaked for 600 hours, and 3) light-soaked followed by annealing at different temperatures. At T = 7 K, the NMR line shape of the sample after light soaking exhibits an additional doublet compared to that of the sample as-grown. This doublet is an indication of a closely separated hydrogen pair. The distance between the two hydrogen atoms is estimated to be about (2.3 ± 0.2) Å. The concentration of these hydrogen sites is estimated to be between 1017 and 1018 cm-3 consistent with ESR measurements of the defect density after light soaking. This doublet disappears after the sample is annealed at 200°C for 4 hours.


2019 ◽  
Vol 484 (1) ◽  
pp. 56-60
Author(s):  
D. A. Indejtsev ◽  
E. V. Osipova

Hydrogen atom behavior in pure aluminum is described by ab initio modelling. All main energy characteristics of the system consisting of hydrogen atoms in a periodic aluminum crystal are found.


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